NASA NTRS · 19720015710
The Gum nebula
Abstract
The distance from the sun to the center of the star, Gamma Velorium, is determined in an effort to draw a physical model and identify the ionized energy source of the Gum nebula. The distance is calculated from the local hydrogen density of radio astronomy studies and the hydrogen measure.
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Brandt, J. C.. 1972-01-01. The Gum nebula. https://ntrs.nasa.gov/citations/19720015710
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